木星 月惑星研究会 関西支部 (最新)
ALPO-Japan Latest
Jupiter Image 2002/03/19(UT)
永長英夫,Antonio Cidadao,Paulo Coelho
H.Einaga,A.Cidadao,Paulo
Hideo Einaga (250mm Newton, Digital Still Camera NEC PICONA)
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2002/03/19 09:27:08 (UT)
CMI = 174.7, CMII = 106.9, CMIII = 203.4
De = +1.9, E.Dia = 39.58"
5 frames composite
Seeing=3/10,Trans=2/5
25cm+barlow3x(F=34)+Picona(1/7s)
2002/03/19 10:27:36 (UT)
CMI = 211.5, CMII = 143.4, CMIII = 240.0
De = +1.9, E.Dia = 39.57"
5 frames composite
Seeing=3/10,Trans=2/5
25cm+barlow3x(F=34)+Picona(1/7s)
2002/03/19 11:23:17 (UT)
CMI = 245.5, CMII = 177.1, CMIII = 273.6
De = +1.9, E.Dia = 39.57"
9 frames composite
Seeing=3/10,Trans=2/5
25cm+barlow3x(F=34)+Picona(1/7s)
HIDEO EINAGA ≪兵庫・加西 永長英夫≫
Antonio Cidadao (280mm C11+ST-237 CCD camera)
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Hi all,
Here are some preliminary images obtained on tonight's session,
unfortunately interrupted by a thick marine fog. Anyway, seeing was
favourable on some occasions and the SSTC WOS (also GRS and BA) longitudes
were well placed for observation.
The "f" pair of the SSTC wos is still very close (closer??; tonight about
6deg center to center in my rough evaluation; on Mar16 my pick was 6.5 deg,
corrected by Hans-Joerg to 5.9 +/- 0.3 degrees). There is still a thin
region of dark material between the two ovals, but with the spatial
resolution that I have been able to reach with my setup and seeing
conditions, it now appears to be vestigial (the small spot that has
appeared some time ago betwen these two ovals looks smaller and hard to
see). As in Mar16 images, the "p" oval of the pair is slightly N of the "f"
oval. I'm very anxious to see more images of these... (my next favourable
window is in two days, weather allowing it; I hope that many of you manage
to get new data during this period!)
The CH4 image continues to show the described appearence for GRS and BA,
and shoes a faint positivity at the SSTC wos. It looks elongated, but there
is not sufficient S/N ratio to get a clear discrimination between two
closely placed spots. CH4 also shows a mid SEB spot in the disturbance "f"
the GRS.
Color and clear images show more elongated and thinner SEBn "feature" (when
compared with previous days). NEB rifts also continue to evolve.
Good observations
Antonio
≪アントニオ シダダオ ポルトガル≫
[Antonio Cidadao Oeiras - Portugal ]
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Paulo Coelho ( 8'' Celestron SCT @ f/28 Toucam Pro Webcam)
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[Montijo, Portugal]
≪パウロ セホ ポルトガル≫
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